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20112023
most citedCosmology in the dark: On the importance of source population models for gravitational-wave cosmology

128 citations · 473 across the 27 of their papers we have counts for

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gr-qc2023★ 17 cited

Entanglement harvesting for different gravitational wave burst profiles with and without memory

Subhajit Barman, Indranil Chakraborty, Sajal Mukherjee

In the present article, we study how different gravitational wave (GW) burst profiles in linearized gravity, with and without the asymptotic memory, may influence the harvesting be…

gr-qc2022★ 8 cited

Transition from inspiral to plunge for braneworld EMRI

Sajal Mukherjee, Sumanta Chakraborty

In the present article, we discuss the late inspiral and then the transition regime to the plunge phase of a secondary, less massive compact object into a more massive braneworld b…

gr-qc2022★ 14 cited

Resonance crossing of a charged body in a magnetized Kerr background: an analogue of extreme mass ratio inspiral

Sajal Mukherjee, Ondrej Kopacek, Georgios Lukes-Gerakopoulos

We investigate resonance crossings of a charged body moving around a Kerr black hole immersed in an external homogeneous magnetic field. This system can serve as an electromagnetic…

gr-qc2021★ 128 cited

Cosmology in the dark: On the importance of source population models for gravitational-wave cosmology

S. Mastrogiovanni, K. Leyde, C. Karathanasis +7

Knowledge of the shape of the mass spectrum of compact objects can be used to help break the degeneracy between the mass and redshift of the gravitational wave (GW) sources, and th…

gr-qc2021★ 3 cited

Thermal behavior of a radially deformed black hole spacetime

Subhajit Barman, Sajal Mukherjee

In the present article, we study the Hawking effect and the bounds on greybody factor in a spacetime with radial deformation. This deformation is expected to carry the imprint of a…

gr-qc2021★ 7 cited

Pure Gauss-Bonnet NUT Black Hole Solution: I

Sajal Mukherjee, Naresh Dadhich

We find a new exact -vacuum solution in pure Gauss-Bonnet gravity with NUT charge in six dimension with horizon having product topology . We also discuss…